Planetary Nebula Luminosity Function

The Planetary Nebula Luminosity Function is a photometric distance indicator that models the statistical distribution of luminosities of planetary nebulae in a galaxy, exploiting their characteristic bright [O III] λ5007 emission to identify a relatively invariant bright-end cutoff usable for estimating extragalactic distances.

176

Publications

11.9K

Citations

429

Authors

230

Institutions

Publications per year

2017–2026

13

Variants

Pnlf

Authors

429

  1. GH
    George H. Jacoby

    Kitt Peak National Observatory, United States

    28 publications · 2.8K citations

    24

    h-index

  2. RC
    Robin Ciardullo

    Pennsylvania State University, United States

    26 publications · 2.5K citations

    23

    h-index

  3. MA
    M. Arnaboldi

    Astronomical Observatory of Capodimonte, Italy

    14 publications · 1K citations

    14

    h-index

  4. OG
    Ortwin Gerhard

    Max Planck Institute for Extraterrestrial Physics, Germany

    12 publications · 823 citations

    12

    h-index

  5. KC
    K. C. Freeman

    Australian National University, Australia

    11 publications · 764 citations

    11

    h-index

1–5 of 429

Venues

  1. The Astrophysical Journal

    ApJ · 64 publications · 4.8K citations

    39

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    22 publications · 1.2K citations

    16

    h-index

  3. The Astronomical Journal

    AJ · 13 publications · 1.7K citations

    13

    h-index

  4. Astronomy and Astrophysics

    14 publications · 772 citations

    12

    h-index

  5. Astrophysics and Space Science

    10 publications · 207 citations

    10

    h-index

1–5